[ 2 9 ] 
35 th Camelopard. 
Hevelii. 
South or 
0 ' 
33. 25 
Precef- 
fion. 
Aberra- 
tion. 
Mutation. 
Mean 
Dill. 
South t 
n 
// 
// 
// 
h 
1727 October 
20 
73.6 
+ 0.9 
- 6.7 
+ 89 
76.7 
1728 Jmuary 
12 
6 o .3 
1.2 
-f- 6.1 
8.8 
7C9 
March 
1 
57.8 
I.4 
-f- 9-4 
8.7 
77-3 
September 
26 
75 - 2 
- 8.8 
8.1 
76.8 
1729 February 
2 6 
56.+ 
2.8 
+ 9-4 
7.6 
76.2 
1730 March 
6 
77.8 
4 4 
9 4 
5.4 
77.0 
1731 February 
5 
59.1 
5.6 
8.5 
-h 3 -o 
7 6 2 
1733 January 
3 1 
64.1 
8.7 
82 
— 2.9 
78.1 
1738 December 
3 ° 
61.8 
17.2 
4-3 
6.5 
76.8 
1739 February 
4 
56.9 
17.3 
3 5 
6.3 
76.4 
174.0 January 
20 
56.0 
18.6 
7 -° 
— 4.0 
77-6 
1747 February 
27 
32.3 
28.7 
9 4 
4- «•+ 
78.6 
The Obfervations of the foregoing Stars arc the 
moll proper, to prove the Change of the Inclination 
of the Earth’s Axis to the Plane of the Ecliptic j 
thofe, which follow, will fncw in what manner the 
Stars, that lie near the Equinoctial Colurc, are af- 
fected, as well as others, that are differently fituated, 
with refpeCt to the Cardinal Points of the Equator. 
Some of thefe Stars are indeed more remote from 
the Zenith, than I would have cholcn, if there had 
been others, of equal Lull re, in more proper Po- 
rtions 5 becaufe Experience lias long fince taught 
me, that the Obfervations of Inch Stars, as lie near 
the Zenith, do generally agree beft wuh one ano- 
ther, and arc therefore the fitted to prove the 
Truth of any Hypothecs. 1 fhall begin with thofe 
near the Vernal Equinox, a CaJJiopex was com- 
pared with the Point masked 34 0 . yy'j and at firft 
was 
